The observed galaxy presents an elongated, lenticular morphology with a noticeable central bulge. The galaxy exhibits a relatively smooth light distribution across its structure, with only subtle indications of spiral arm features. The central bulge appears bright, with intensity gradually decreasing towards the outer regions. Slight asymmetry in the disk suggests a possible minor gravitational interaction or past merger event. The galaxy color index suggests a population of older stars, particularly in the central bulge. There are no distinctly visible star-forming regions. Overall the galaxy appears to be a mature system with relatively low star formation activity.
