The galaxy presents as a roughly elliptical form, exhibiting a smooth, diffuse appearance with a centrally concentrated bulge. The color profile suggests a mature stellar population, with a subtle redder hue towards the core and a slightly bluer tinge in the outer regions. There are indications of some minor disturbances in the outer arms, possibly resulting from gravitational interactions, although no clear merging activity is immediately apparent. Overall, the galaxy appears to be an intermediate mass, with a low-to-moderate star formation rate. The light distribution is centrally condensed, with an overall smooth morphology suggesting a classification towards the elliptical side of the Hubble sequence. The overall structure is suggestive of an older galaxy.
