The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its morphology indicates characteristics of an early-type galaxy, possibly an elliptical or lenticular, showing little to no discernable spiral arm structure. The central region exhibits a brighter, more condensed core, suggesting a higher density of stars. The galaxy's color profile appears to be relatively uniform throughout, with a slight tendency towards redder hues, particularly in the outer regions, suggesting a relatively older stellar population and low star formation activity. There is minimal visual evidence of ongoing major mergers or significant tidal disturbances. However, subtle irregularities in the light distribution could indicate minor interactions or past merger events.
