The galaxy appears as a concentrated, luminous structure with a primarily smooth morphology. Its overall shape is somewhat elliptical, exhibiting a tendency toward roundness rather than a highly elongated form.

The central region displays the highest surface brightness. The color profile suggests a dominant population of older stars, consistent with a relatively low star formation rate. There are no prominent spiral arm features, bars, or other signs of strong galactic disk activity visible in the image. There are some signs of possible interactions with a small number of very faint nearby sources, although these are not clear merger events. 
