This galaxy appears to be an elliptical or lenticular galaxy, exhibiting a generally smooth and symmetrical morphology. There is an observed elongation, indicating a cigar-shaped structure. The galaxy displays a concentration of light in its central region, gradually decreasing outwards. The color profile suggests a slightly older stellar population, shifting toward redder hues. There's no clear evidence of ongoing major star formation, or significant dust lanes. Tidal features or other signs of a recent major merger event are not readily apparent, although there may be some minor disturbances.
