The galaxy presents as an elongated, cigar-shaped structure with a prominent central bulge. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color profile transitions from a yellowish-white in the core to a redder hue towards the outer edges. The galaxy appears relatively smooth in texture, lacking any distinct spiral arm structures or prominent dust lanes. Faint, diffuse extensions of light are observed, but these are not well-defined. There is no strong indication of any ongoing major merger activity or significant tidal disturbances. The overall appearance suggests a system dominated by an older stellar population, with limited recent star formation.
