The galaxy presents an elliptical morphology, appearing largely smooth and featureless in this observation. The light distribution suggests a centrally concentrated spheroid, with a gradual decline in luminosity towards the outer edges. The core region displays a yellowish hue, potentially indicative of an older stellar population. The overall color profile leans towards the redder end of the spectrum. The structure suggests a lack of significant ongoing star formation. A slight elongation is visible, deviating from a perfectly circular shape. There is no obvious evidence of spiral arms, dust lanes, or prominent star-forming regions. No signs of tidal disturbances or interactions with other galaxies are immediately apparent, implying relative isolation, a merging event cannot be ruled out completely.
