The galaxy presents as a moderately bright object with an apparent, though somewhat indistinct, elliptical morphology. The central region exhibits a high degree of luminosity, suggesting a significant concentration of stars and possibly an active galactic nucleus. The light distribution transitions gradually from the core, indicating a relatively smooth stellar population profile. There appears to be a slight color gradient, with the central region presenting a more yellow-red hue, potentially due to a larger population of older stars or increased dust extinction. A subtle hint of possible interaction or minor disturbance is suggested by a faint, extended feature to the upper right. Otherwise, the overall appearance suggests a relatively evolved system, likely with moderate star formation activity and a significant stellar mass. The galaxy has a round shape, rather than cigar-shaped, and may not be undergoing any major mergers.
