The observed galaxy presents as a relatively smooth, elliptical structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. No distinct spiral arms or prominent dust lanes are discernible. The galaxy exhibits a yellowish-red color, potentially indicating a population dominated by older stars and a lower rate of ongoing star formation. The overall shape suggests a near-spherical morphology, with a slight elongation. There is no evidence of significant tidal disturbances or interactions with other galaxies in the immediate vicinity.
