The galaxy presents as an elongated, somewhat diffuse object. Its overall shape is consistent with an elliptical galaxy viewed from an oblique angle. There is a pronounced central bulge region which appears smoother and more concentrated. A disk-like structure is also visible, and is oriented nearly edge-on relative to our line of sight. Within the disk component, there are subtle indications of spiral arm-like features. The galaxy's color profile suggests a mixed stellar population. The central region exhibits a yellowish hue indicative of older, redder stars. The disk regions display a bluer tint, implying the presence of younger, hotter stars and potentially ongoing star formation. No strong dust lanes or prominent star-forming regions are immediately apparent, but some subtle clumpy features can be seen within the bluer regions of the disk. The galaxy appears to be relatively isolated, without obvious signs of tidal interactions or major mergers occurring. The image data quality limits detailed morphological characterization, further analysis is warranted.
