This galaxy exhibits an elongated, cigar-shaped morphology. The central region appears bright and concentrated, indicating a substantial bulge component, likely populated by older stars. The color gradient suggests a redder hue in the core, consistent with an older stellar population and potentially a supermassive black hole accreting mass in the center. Moving outwards from the core, the light becomes slightly bluer. The edges are quite indistinct which could be from galactic dust and gas. There are no apparent spiral arm structures or prominent dust lanes and there is no indication of a major merger. It likely hasn't been significantly disturbed by interactions with neighboring galaxies. Overall, it seems to be a relatively quiescent galaxy, with likely lower star forming properties.
