The galaxy presents a distinct elongated morphology, appearing cigar-shaped. The light distribution is generally smooth, with a dominant central bulge that appears relatively featureless. There's a slight hint of a disk component, but it is not clearly defined and might be a pseudodisk. The galaxy exhibits a redder hue, possibly suggesting a population of older stars and/or significant dust obscuration. No prominent spiral arms or distinct star-forming regions are discernible. There is no strong evidence of tidal disturbances or ongoing major merging activity, although the elongated shape could suggest past interactions or minor disturbances. Overall, the galaxy appears to be a relatively evolved system with a dominant spheroid component.
