The galaxy presents as a relatively compact object, elliptical in shape, with an apparent deviation from perfect sphericity towards a slightly elongated, cigar-like form. Its dominant color is a pale blue hue, suggestive of a population of young, hot stars and potential ongoing star formation within the galaxy. The light distribution appears smooth, with no readily discernible spiral arms or prominent dust lanes. There is no clear visual evidence of tidal tails or significant morphological disturbances indicative of recent major merger events, although subtle irregularities cannot be ruled out. Overall, the galaxy appears as a fairly isolated, undisturbed system.
