The galaxy presents as a slightly elongated, elliptical structure with a smooth, featureless appearance. The central region exhibits a concentrated luminosity gradient, indicating a prominent bulge. The color profile suggests an older stellar population, with a yellow-orange hue dominating the central region, possibly indicative of reduced recent star formation. There is some asymmetry in the outer regions of the galaxy which may point to signs of a minor disturbance or interaction.  The morphological classification appears to be that of an elliptical galaxy, viewed at an oblique angle.
