The galaxy presents as a relatively smooth, elliptical morphology. The object exhibits a somewhat elongated shape, with a clear color gradient. The central region of the galaxy appears bright and yellow, possibly indicative of an older stellar population or dust obscuration, with a faint, diffuse halo extending outwards. The smooth morphology suggests a lack of significant recent star formation. The overall light distribution is concentrated in the core with a gradual decrease in intensity toward the edges. There are no discernable spiral arms or prominent dust lanes visible within the resolution limits. The overall appearance indicates a galaxy undergoing or having completed the transition to a passive, redder state. There might be a second galaxy in the process of merging with this galaxy.
