The galaxy presents as a relatively smooth, elliptical form, with an apparent lack of spiral arm structures or prominent dust lanes. Its color profile indicates a dominant population of older stars, exhibiting a yellowish-orange hue concentrated towards the galactic center, possibly suggesting a higher density of these stars within the core. There may be a small, irregular galaxy merging on the left side of the primary galaxy. There is no clear indication of recent major starburst activity. The galaxy appears to be generally undisturbed, without any obvious signs of tidal tails or distortions indicative of recent major mergers, although there is a possible sign of minor disturbance in the merging galaxy.
