The galaxy presents as a moderately bright, relatively compact object. The light profile appears smooth and largely featureless, suggestive of an elliptical or lenticular morphology. The central region exhibits a yellowish hue, possibly indicating an older stellar population. Surrounding this core, a more diffuse, bluish halo can be observed, indicative of a younger, hotter stellar population and/or ongoing star formation at a low rate. There is no strong evidence of spiral arms or a well-defined disk structure in this image. The overall shape is mostly round, but it is not perfectly circular. There is potential evidence of minor disturbances in the galaxy’s morphology, such as a slight asymmetry or faint tidal features, suggesting a possible recent or ongoing interaction with another galaxy.
