The galaxy exhibits a predominantly smooth morphology with a bright, concentrated central bulge. The radial color gradient suggests a population of older stars dominating the core, transitioning outwards to bluer hues, possibly indicative of younger stellar populations in the outer regions. There is a subtle hint of disk-like structure, although the lack of defined spiral arms suggests a classification towards a lenticular galaxy or a disk galaxy with low surface brightness spiral arms. A small portion of the galaxy shows slight asymmetry, perhaps indicating a very minor tidal interaction or ongoing accretion event. Overall, the galaxy presents as relatively isolated with no major signs of an ongoing merger event. The presence of a potential minor disturbance could indicate a minor interaction, but the galaxy appears largely undisturbed.
