The galaxy presents as a somewhat elongated, yet generally smooth structure. The central region exhibits a concentrated luminosity, appearing significantly brighter and with a yellowish hue, suggesting a population of older stars. Moving outwards from the center, a gradual decrease in surface brightness is observed. There is a subtle extension of the galaxy along its major axis, giving it a slightly cigar-shaped appearance, but there are not apparent distinct spiral arms or other defined features. The overall color profile indicates that this galaxy might be undergoing some level of star formation activity, but it is likely subdued. There is a subtle disturbance or asymmetry visible in the outskirts, possibly indicative of a minor interaction or past merger event, though more detailed imaging would be needed to confirm this. The galaxy appears to be relatively isolated within the field of view.
