The galaxy presents as an elliptical morphology, characterized by a centrally concentrated luminosity profile. The core region exhibits a bright, yellowish hue, possibly indicative of an older stellar population. There appears to be a gradual decrease in surface brightness from the core outward, with no distinct spiral arms or prominent dust lanes visible. The overall structure suggests a relatively smooth and symmetrical distribution of stellar material. There is no apparent significant tidal distortion or interaction with neighboring galaxies based on visual inspection. The galaxy's color profile hints at a evolved stellar population and a low ongoing star formation rate.
