The galaxy presents as a generally smooth, centrally concentrated object with a slightly elliptical morphology. The central region exhibits a bright, yellowish hue, suggesting a population of older stars. There is little evidence of prominent spiral arms or distinct features typically associated with actively star-forming galaxies. A subtle color gradient is observed, with the central region appearing yellower compared to the outer regions, which have a slightly bluer tint. This might indicate some ongoing, albeit low-level, star formation in the outer disk. There appears to be a very minor, faint disturbance that could be the result of a minor merger, though it is subtle and could also be internal. The galaxy is somewhat rounded, but slightly elongated, resembling an intermediate shape between perfectly spherical and a cigar-like form. Overall, the galaxy appears to be a relatively quiescent system.
