The galaxy presents as a relatively compact, bright central region, suggestive of a substantial bulge component. Its color gradient shifts from a yellow-white core, potentially indicative of an older stellar population, to slightly bluer hues in the surrounding regions, implying more recent star formation activity. The overall structure appears disturbed, with a subtle, possibly faint disk component. There is a slight asymmetry, with a hint of tidal features or faint arms, suggesting a past or ongoing minor interaction or merger event. The shape leans towards a more elliptical morphology, though the disturbed features complicate this classification.
