The galaxy presents as a centrally concentrated object with a bright, unresolved core. The overall shape is generally elliptical but displays some irregularities in its outer regions, suggesting a possible deviation from a perfect elliptical form. The color profile indicates a predominantly older stellar population, with a subtle blue tinge in the outer disk, hinting at ongoing, albeit modest, star formation. There appears to be a smooth transition between the core and the outer regions. The galaxy exhibits signs of a minor disturbance, potentially indicating a past or ongoing interaction with another galaxy, or perhaps internal dynamics affecting its structure.
