The galaxy exhibits a generally smooth morphology, suggesting a classification toward the elliptical end of the Hubble sequence. It is characterized by a centrally concentrated luminosity profile that decreases gradually towards the edges. The object is elongated, approximately cigar-shaped, rather than perfectly spherical. There is no discernible spiral arm structure or dust lane features in the image. The galaxy appears to be a yellowish hue, possibly indicative of an older stellar population. There are no obvious signs of tidal disturbances or ongoing major merging events. A minor degree of disturbance cannot be excluded, but the overall structure does not present indications of significant interaction history. The size appears moderately large, consistent with a galaxy of considerable stellar mass.
