This galaxy presents as an elongated, cigar-shaped structure, suggestive of an elliptical morphology. The central region exhibits a high degree of luminosity, appearing as a concentrated and relatively smooth distribution of light. Progressing outwards from the core, the light intensity gradually diminishes into a diffuse halo. While there are some vague indications of a disk, there is no clear presence of spiral arms or prominent dust lanes within this galaxy. The overall color is consistent with a population of older stars. There is no apparent strong star forming regions or recent merger events.